A review is made of supernovae, supernova remnants and pulsars, with particular reference to the Vela X SNR and PSR0833-45. A detailed description is made of two experiments built and flown on a Skylark sounding rocket. One of these made a one-dimensional scan of the Vela X and Puppis A SNRs in the energy range 0.2--2 KeV. The second experiment sought pulsed emission from PSR0833-45 in the energy range 1.3--13 KeV. The results of the above experiment are presented, including one-dimensional profiles and upper limits to pulsed emission. Finally, data is presented from the observations of the general Vela region by the Sky Survey Instrument on board the Ariel V satellite. In particular, a synchrotron x-ray emitting region about 2 in diameter ...
The Vela supernova remnant (SNR) is a complex region containing a number of sources of non-thermal ...
SIGLECopy held by FIZ Karlsruhe; available from UB/TIB Hannover / FIZ - Fachinformationszzentrum Kar...
International audienceThe Vela pulsar (PSR J0835 − 4510) is the brightest persistent source in the h...
A review is made of supernovae, supernova remnants and pulsars, with particular reference to the Vel...
A soft X-ray observation of the Vela Supernova Remnant is described. X-ray surface brightness maps ...
Open Access. Supernova remnants and their X-ray emission; Proceedings of the Symposium, Venice, Ital...
The Vela pulsar was observed in the range 2-60 keV by the GSFC proportional counter experiment onboa...
A review of X-ray observations in the vicinity of the Gum nebula is presented. There is little doubt...
The Vela supernova remnant is the closest SNR to contain a young active pulsar, PSR B0833-45. The re...
Supernova Remnants (SNRs) are believed to be acceleration sites of Galactic cosmic rays. Therefore, ...
Pulsars are known to power winds of relativistic particles that can produce bright nebulae by intera...
One of the best objects for study of the structure, kinematics, and evolutionary status of a middle-...
5 pages, 4 figures, accepted for publication in Astronomy and Astrophysics lettersThe Vela supernova...
We have observed the Vela pulsar region at TeV energies using the 3.8 m imaging Cerenkov telescope ...
The Vela supernova remnant (SNR) is a complex region containing a number of sources of non-thermal ...
SIGLECopy held by FIZ Karlsruhe; available from UB/TIB Hannover / FIZ - Fachinformationszzentrum Kar...
International audienceThe Vela pulsar (PSR J0835 − 4510) is the brightest persistent source in the h...
A review is made of supernovae, supernova remnants and pulsars, with particular reference to the Vel...
A soft X-ray observation of the Vela Supernova Remnant is described. X-ray surface brightness maps ...
Open Access. Supernova remnants and their X-ray emission; Proceedings of the Symposium, Venice, Ital...
The Vela pulsar was observed in the range 2-60 keV by the GSFC proportional counter experiment onboa...
A review of X-ray observations in the vicinity of the Gum nebula is presented. There is little doubt...
The Vela supernova remnant is the closest SNR to contain a young active pulsar, PSR B0833-45. The re...
Supernova Remnants (SNRs) are believed to be acceleration sites of Galactic cosmic rays. Therefore, ...
Pulsars are known to power winds of relativistic particles that can produce bright nebulae by intera...
One of the best objects for study of the structure, kinematics, and evolutionary status of a middle-...
5 pages, 4 figures, accepted for publication in Astronomy and Astrophysics lettersThe Vela supernova...
We have observed the Vela pulsar region at TeV energies using the 3.8 m imaging Cerenkov telescope ...
The Vela supernova remnant (SNR) is a complex region containing a number of sources of non-thermal ...
SIGLECopy held by FIZ Karlsruhe; available from UB/TIB Hannover / FIZ - Fachinformationszzentrum Kar...
International audienceThe Vela pulsar (PSR J0835 − 4510) is the brightest persistent source in the h...